CWWDL 14359

0.02 UTI

0.42

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.05

C_dup

C3 classification AA

Number of members (P>50%) 42

Radius (P>50% members) 7.8 [arcmin]

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14359 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14359 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	277.015	-15.357	0.868	-2.67	-3.594	16.412
Chi et al.	2023	277.025	-15.382	0.88	-2.644	-3.673	21.956

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Chi et al.	2023	–	–	–	29	0.230	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 57	95.2	276.99	-15.35	0.87	-2.67	-3.57	12.94	0.18
Theia 2510	92.9	277.01	-15.36	0.87	-2.66	-3.57	12.94	0.0
PHOC 20	76.2	277.0	-15.39	0.87	-2.67	-3.59	16.41	0.43

💡 Note: The % column shows the percentage of members that CWWDL 14359 shares with each listed object.

Visualization

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